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Solar Orbiter Study Finds Large Solar Flare Triggered by 'Magnetic Avalanche'

High-cadence, multi-instrument observations reveal a cascading reconnection engine that reshapes flare models and points to a need for higher-resolution X‑ray data.

Overview

  • Peer-reviewed results published January 21, 2026 in Astronomy & Astrophysics analyze a major flare recorded during Solar Orbiter’s September 30, 2024 close pass.
  • EUI, SPICE, STIX and PHI captured complementary layers from corona to photosphere, resolving features a few hundred kilometers wide and changes every two seconds.
  • Roughly 40 minutes of precursor activity showed many small reconnection events that spread rapidly in space and time and collectively drove the large eruption.
  • Measurements documented a detached filament, bursts of brightness, streams of raining plasma blobs, and particles accelerated to about 40–50% of light speed.
  • Researchers say the case study challenges existing flare-energy-release models, informs space-weather understanding, and requires further events plus sharper X‑ray imagery to test how universal the mechanism is.